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The Evolution of The Milky Way pp 291–300Cite as

Abundances of Globular Clusters in the Galactic Bulge

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 255))

Abstract

Element ratios in two stars of NGC 6553 and one star in NGC 6528 reveal that a-elements are enhanced relative to Fe. The metallicity [Fe/H] -0.5 combined to overabundances of several elements gives an overall metallicity close to solar for both clusters

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Author information

Authors and Affiliations

  1. IAG/USP, São Paulo, Brazil

    B. Barbuy

Authors
  1. B. Barbuy
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Editor information

Editors and Affiliations

  1. Dipartimento di Astronomia, University of Trieste, Italy

    Francesca Matteucci

  2. Instituto di Astrofisica Spaziale, Fuescoti, Italy

    Franco Giovannelli

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© 2000 Springer Science+Business Media Dordrecht

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Barbuy, B. (2000). Abundances of Globular Clusters in the Galactic Bulge. In: Matteucci, F., Giovannelli, F. (eds) The Evolution of The Milky Way. Astrophysics and Space Science Library, vol 255. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0938-6_29

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  • DOI: https://doi.org/10.1007/978-94-010-0938-6_29

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-3799-0

  • Online ISBN: 978-94-010-0938-6

  • eBook Packages: Springer Book Archive

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